Since the discovery of neutrino oscillations, we know that neutrinos have non-zero mass. However, the absolute neutrino-mass scale remains unknown. Here we report the upper limits on effective electron anti-neutrino mass, mν, from the second physics run
In this paper we develop the formalism needed for doing noncommutative geometry with operator systems. We will focus mainly on the ‘topological properties’ described by the operator systems and corresponding state spaces. The metric aspect as provided by spectral triples extends in a straightforward ...
This obtained result was in accordance with the research of Kannah et al., (2017) in which phase separation was noticeable at 3,000 rpm within 30 sec at the shear force of 104.25 G force. Beyond the disperser time of 30 s and shear force, the cell cleavage occurs stimulating the sludge...
I experienced his predecessor’s, George Withbroe’s, unexpectedly angry retort when I suggested in a Roadmap meeting at NASA/HQ that a mission to monitor the entire Sun in a variety of wavelengths would be of great value to SEC: “We do science at NASA! We do not ‘monitor’!” Bei...
3. Method In this section, we first give the overall framework of our proposed physics-augmented autoencoder (PAA) in Sec. 3.1. Then we introduce the graph-convolution-based encoder and physics-based decoder in Sec. 3.3 and Sec. 3.4 respectively. The details of ...
3−3mm were used, and time steps between Δ0.01−Δ0.1sec without a significant degradation in prediction quality. The effects of experimental noise were also tested in this study, and the network demonstrated excellent robustness when Gaussian noise was added to the training data. A key ...
The time needed for 129 collision is 129 collision/0.13 collision per sec ∼990 s. In that time, the proton will be ∼58 RM down in the anti-sunward direction of Mars. If we use the average potential value of ∼0.08 V that compensates for the effects of the finite sensor ...
In this research, we study traveling wave solutions to the fractional extended nonlinear SchrÖdinger equation (NLSE), and the effects of the third-order dispersion parameter. This equation is used to simulate the propagation of femtosecond, plasma phy
6 show the effectiveness of our proposed strategy in Sec. 3.4. 5. Conclusion In this paper, we proposed a novel physics-guided ISO- dependent sensor noise model for modeling real rawRGB noises in extreme low-light scenes and collected an LLD dataset unde...
With this in mind, in this sec- tion, we (1) present the proposed physics-informed deep learning method as a novel, non-intrusive ML-based MOR method, (2) show the differences from the existing non- intrusive ML-based MOR methods, e.g., [40,64], and (3) demonstrate how the ...